X-ray FE line studiesWe present the first broadband, moderate-resolution X-ray spectral observations of the Seyfert galaxies NGC 4151 and NGC 1068. The Seyfert 1 galaxy NGC 4151 is shown to have a complex X-ray spectrum with multiple components and a strong, intrinsically narrow Fe K emission line. The characteristics of the scattering medium of the Seyfert 2 galaxy NGC 1068 are determined using the very strong Fe line emission and the lack of features due to oxygen in the X-ray spectrum. The soft X-ray flux from Mrk 3 and Mrk 348 are consistent with that expected from electron scattered X-rays from an obscured Seyfert 1 nucleus. A survey of the X-ray properties of Seyfert 2 galaxies indicates that a substantial fraction may have column densities of about 10 exp 23, suggesting that NGC 1068 has an unusually thick obscuring torus.
Document ID
19930045828
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Marshall, F. E. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Arnaud, K. (NASA Goddard Space Flight Center Greenbelt; Maryland Univ., College Park, United States)
Boldt, E. A. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Holt, S. S. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Jahoda, K. M. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Kelley, R. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Mushotzky, R. F. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Netzer, H. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Petre, R. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Serlemitsos, P. J. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 16, 2013
Publication Date
January 1, 1992
Publication Information
Publication: In: Testing the AGN paradigm; Proceedings of the 2nd Annual Topical Astrophysics Conference, Univ. of Maryland, College Park, Oct. 14-16, 1991 (A93-29801 11-90)